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Ch 29 The Sun Review

AB
Nuclear Fusionnuclei of small atoms combine to form a different atom with the release of energy.
Radiative Zonesurrounds the core where energy moves outward from atom to atom to form electromagnetic waves or radiation.
Convective zonesurrounds the radiative zone area where energy is carried upward by movement of gases as hot gases rises and cool gases sinks.
Photospherevisible surface of the sun.
Chromospherelies above the photosphere reddish in color due to hydrogen.
Coronaoutermost layer of the atmosphere.
Corecenter of the sun where nuclear fusion occurs fusion of hydrogen into helium 15 million degrees Celsius hottest area.
Prominencea loop of cooled gas that extends above the photosphere flow along magnetic curved lines from of one polarity to opposite polarity.
Solar flarean explosive release of energy.
Aurorainteraction when solar wind reaches Earth's magnetosphere produced bands of colored lights.
Solar Windelectorally charged particles thrown off from the sun that travels outward in space.
Coronal mass ejectiongas from the corona that is very violently ejected or thrown into space.
E=mc2law of relativity
Eequals energy
mequals mass or amount of matter used
cequals the speed of light
convectionhot gas rise and cooler gas sinks


Instructional, Schoology, Digital Tools, and AVID Support Tech
Maya Angelou Community High School
Los Angeles, CA

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